- Research article
- Open Access
Non-invasive identification of paint binders in illuminated manuscripts by ER-FTIR spectroscopy: a systematic study of the influence of different pigments on the binders’ characteristic spectral features
Heritage Sciencevolume 7, Article number: 7 (2019)
This paper presents the results of a study of pigment-binder systems painted on parchment, both in the form of reference samples prepared in the laboratory, and of medieval and Renaissance illuminated manuscripts, by means of contactless Fourier-transform mid-infrared spectroscopy (FTIR). The research is aimed at validating external reflection FTIR (ER-FTIR) as a non-invasive method for the identification of paint binders in works of art on parchment. Based on a systematic FTIR investigation undertaken both in attenuated total reflection (ATR) and ER mode, we discuss the possibility to effectively discriminate between different binders, and the way in which the presence of a number of pigments can modify the spectral features of the pigment-binder system. The study reveals that gum Arabic can usually be discriminated from egg-based binders such as egg yolk and egg white, both in paintouts and in real artworks. Amongst all the pigments investigated, carbonates such as azurite and lead white are those that most significantly hinder the correct identification of the paint medium.
Infrared spectroscopy is a well-established and widely used analytical technique in the heritage science field. The reasons of its success are to be found both in its wide applicability and in the significant instrumental developments from the 1970s to this day. By the 1980s, infrared spectroscopy had ‘become an invaluable and extremely flexible tool for the analysis of nearly all artistic materials, from the classic to contemporary ones’ . The last thirty years have seen this trend confirmed, as the number of publications concerning the application of FTIR spectroscopy to the study of heritage materials has grown dramatically. The strength of mid-infrared spectroscopy has traditionally lied not only in its ability to recognize classes of compounds but also in the small amount of material that is needed for the analysis. In the last two decades however, the development of portable, contactless, FTIR spectrometers operating in external reflection, has also allowed the beginning of non-invasive mid-infrared spectroscopy analyses on cultural heritage materials [2 and references therein]. ER-FTIR is totally non-invasive because it does not require sampling or even contact with the object, which can be placed a short distance (approximately 1 mm) from the instrument. The instrumentation is often portable and therefore suitable for in situ analysis, which is a definite advantage for the study of artworks. Another benefit consists in the possibility to collect spectra in a broad spectral range, which includes the near-infrared (7500–400 cm−1, i.e. 1330–25,000 nm). Despite its versatility, ER-FTIR shows a significant drawback in the spectral interpretation. The complexity of the spectra, in the form of bands distortions and variations of their intensity ratio, is ascribable to the specular (Rs) and volume (Rv) components of the reflected radiation. While the former causes derivative-like distortions in the band shape and/or band inversion (reststrahlen effect), the latter enhances the intensity of the weakest bands, such as overtones and combination bands. Since both the physical properties (e.g. morphology, particles size, surface roughness) and the optical properties (absorption and refractive indices) of the substrate can influence the penetration of the incident radiation, the spectral features will be affected by the different contribution of Rs and Rv. Such spectral distortions are usually not present, or evident, in FTIR spectra collected in attenuated total reflection mode (both in ATR or micro-ATR mode); this approach, however, requires either a microscopic sample or the application of significant pressure on the surface under analysis, and is therefore often not suitable for the analysis of works of art. In the majority of cases, ATR spectra can be interpreted by (automated) comparison with spectral databases, which are usually sold with the instrument itself. This is not usually possible with spectra collected in ER-FTIR mode.
While the ATR and μ-ATR are widely used in the characterization of Illuminations and manuscripts [3,4,5,6], the use of ER-FTIR is still limited [7,8,9]. The main goal of the present study is the evaluation of the possibility to discriminate the different classes of binders, e.g. lipids vs. proteins vs. carbohydrates, when they are mixed with different pigments. In particular, we focused our attention on the influence of the pigments’ vibrational features on the position and distortion of the organic binder’s marker bands. The use of organic binders, with good filmogenic properties, often produces very smooth pictorial layers, in which the inorganic pigments are embedded. In terms of reflection, the smoothness of the surface enhances the RS component, and in the case of inorganic pigments such as carbonates, the result is the appearance of intense reststrahlen bands . The superposition between inverted absorption and derivative-like distorted bands, typical of organic compounds, can give rise to very complex spectra. To understand how pigments can influence the marker bands’ position, a preliminary comparison among μ-ATR and ER-FTIR spectra was performed. About 100 paintouts on parchment, representative of pure binders and pigment-binder systems, were studied. These paintouts were designed to replicate the structure of paint layers on western European manuscripts produced during the Middle Ages and the Renaissance. Before discussing the discrimination among different binders and/or pigments, the spectral features of the samples prepared by painting each pure binder over parchment are presented, and their vibrational bands attributed to specific functional groups. As mentioned, ER-FTIR spectra can differ substantially from those collected in other configurations, including ATR mode. This can be very well illustrated by a comparison of ER-FTIR and ATR spectra of pure binders painted on parchment, which also facilitates the attribution of absorption bands identified in the ER-FTIR spectra. After a thorough review of the paint layers’ spectral features, selected areas were also analysed in a number of manuscript cuttings and bound volumes.
Materials and methods
The paintouts were prepared by brush coating natural parchment with different pigment/binder mixtures. Each pigment was bound with four different paint binders, chosen to simulate mediaeval and Renaissance illuminations: gum Arabic (GA), egg yolk (EY), egg white (albumen, EW) and whole egg (WE) were chosen. The pigments were also chosen to span the colour range of those most widely used in illuminations and included blue (azurite, ultramarine, indigo and smalt), yellow (lead–tin yellow I), red (vermilion, red lead, madder lake, lac lake), white (gypsum, chalk, lead white) and green (malachite, verdigris, green earth) ones. The paintouts’ thickness was not directly measured, but based on similar lab-made samples, the paint layers are estimated to be between 10 and 200 microns thick.
Infrared spectra were acquired using a portable contactless Bruker Alpha spectrometer operating in the 7500–400 cm−1 range. Forty scans, with a resolution of 4 cm−1, were performed for each measurements and the analysed area was around 5 mm in diameter. Micro-ATR spectra were collected on the paintouts using a Spectra Tech Continuum optical microscope, mounting a Si ATR objective, coupled to a Thermo Scientific Nicolet iS 10 and equipped with an MCT detector. The spectra (64 scans) were collected in the 4000–650 cm−1 range with a resolution of 4 cm−1. As is well known , spectra collected in external reflection mode can be extremely different from those collected in transmission mode. The attribution of spectral bands to specific vibrational modes was therefore based on a comparison with the spectra collected in μ-ATR mode. The presence of derivative-like distortions or inverted bands was evaluated case by case, taking into account the complexity of the spectrum and the physical nature of the paint film. Due to the chemical and physical heterogeneity of the investigated sample, the Kramers–Kronig transformation was not applied. The spectra were only smoothed using the Savitzky Golay algorithm available in the instrument’s own spectral acquisition software.
Results and discussion: paintouts
The parchment support, prepared by processing animal skin, is mainly composed of collagen, a polypeptidic material which gives rise to two characteristic amide bands, amide I (hereafter AI) and amide II (hereafter AII). According to the literature [5, 10], AI and AII are centred at 1693 and 1547 cm−1 respectively in the μ-ATR spectrum, whereas in ER-FTIR they both show a typical derivative-like distortion, with the inflection points centred at 1662 and 1555 cm−1 respectively (Fig. 1a). Also the N–H stretching, whose shape and position are well-defined in μ-ATR spectrum, appears distorted and weakened in intensity in the ER-FTIR spectrum. In the 4000–6000 cm−1 region, one finds a distinctive absorption for proteinaceous material, that is the ν + δ(N–H) combination band  centred at ≈ 4890 cm−1. The AI, AII and ν + δ(N–H) combination bands will therefore be markers not only for parchment but also for any pure proteinaceous binder, such as egg white.
Pure binders on parchment: ATR vs. ER-FTIR spectra
Due to the glossy nature of the gum Arabic layer, the GA ER-FTIR spectrum (Fig. 1b) is dominated by the strong and distorted bands—both stretching (ν(OH)) and bending (δ(OH))—of the hydroxyl functional groups in polysaccharide units. The former, centred at 3320 cm−1 in the μ-ATR spectrum, appears to be distorted, with clear derivative features, showing an inflection point at ≈ 3350 cm−1. The latter, centred at 1604 cm−1 in the μ-ATR spectrum, presents a broad absorption, partially affected by derivative distortion, in the 1900–1600 cm−1 range. The absorption broadening can be attributed to the overlap between the distorted δ(OH), with an inflection point at ≈ 1604 cm−1, and a carboxylate stretching band, present as a shoulder in the μ-ATR spectrum (≈ 1643 cm−1). The presence of νCOO− band can be representative of a partial hydrolysis of the polysaccharide units.
The ν(C–O) of the glycosidic bond displays an intense inverted band at 1020 cm−1. In the spectral region above 4000 cm−1, the absorption features are due to combination bands and overtones of the principal vibrational modes of the polysaccharide structure. They are, however, often superimposed with those originating from the substrate (parchment) and/or too broad and weak to be useful diagnostic tools. When trying to distinguish gum Arabic from other binders, the ν(OH) band also cannot be used as a characteristic marker, because it is often overlapped by the NH and/or OH stretching absorptions typical of the investigated materials (i.e. parchment and pigments). However distorted, it is the band assigned to δ(OH) that can be used reliably to distinguish gum Arabic from the other binders studied here.
Egg based binders, i.e. egg yolk, egg white and whole egg show rather complex spectra, with variations depending both on the chemical and on the physical features of the paint layer (Fig. 1c–e). The main chemical difference between these three binders is the fact that EW is a purely proteinaceous binder, whereas EY and WE also contain a lipidic fraction. Their spectra will therefore show, in addition to the two amide bands, also the lipid features. Generally speaking, the presence of a lipidic component can be easily detected by the intense C=O asymmetric stretching and by the typical ν + δ(CH) combination bands . The former usually displays a feature with a typical derivative-like shape, detectable in the 1800–1700 cm−1 range. Usually broad but well defined, it is centered around ≈ 1740 cm−1 when the derivative distortion component is low. The latter, undistorted and centered at 4399 and 4266 cm−1, are well distinguishable in both pure EY (Fig. 1c) and WE (Fig. 1e), as well as in most of the binder/pigment systems, as will be discussed later. It is worth noting that also the broad band at ≈ 5800 cm−1, due to the first overtone of the CH2 asymmetric stretching, is typical of natural lipid-containing binders; it can be used to support our attribution. For all three egg-based binders, the amide I and II bands are located at approximately 1693 and 1560 cm−1, respectively. Common to all proteinaceous materials, the N–H stretching bands, between 3360 and 3660 cm−1, are not well detectable in egg-based binders and can therefore not be easily used as markers for their identification.
Overall, these observations suggest that—at least in these simple ‘model’ systems—distinction amongst these four different binders painted on a parchment support is usually possible using ER-FTIR spectroscopy, thanks to the presence of specific ‘marker’ bands: GA is easily distinguishable from egg-based media; EY can be further discriminated from EW because of its lipidic content (Fig. 2). WE, however, can easily be confused with EY or with EW, depending on the presence or absence of the characteristic absorption bands of lipids in the individual spectrum, which in turn depends on the lipidic fraction concentration in the sample. It is worth observing that, if the binder layer is very thin, the signals due to the substrate can also be identified, because—depending on the specific features of each individual sample—the incident radiation can penetrate the sample up to a depth of several tens of microns. With the exclusion of EW, the parchment’s absorption, however, does not significantly affect the intensity and shape of the main absorptions due to the pure binders, as measured on samples of binders painted on glass slide (spectra not shown). Only the ν + δ(N–H) at 4880 cm−1 is observed in particularly thin GA paints. Also a broadening in the O–H stretching region, due to the superimposition of the intense signals of both substrate and paint binders, is sometimes observed.
As already mentioned, the paintouts were also investigated by μ-ATR, in order to understand how the ER configuration modifies the IR spectral features. During that experiment we observed that μ-ATR spectra are not always representative of all the functional groups present in the paint layer. This behavior is related to the physical properties, i.e. hardness and/or rigidity, of the paint film, and with the fact that the μ-ATR crystal needs to be in ‘intimate’ contact with small portion of the sample surface (≈ 50 μm2) in order to obtain a spectrum. Such close contact is achieved by applying a significant pressure on the sample. If the film is brittle, as was found to be the case for EW and WE, the applied pressure is high enough to induce fractures and de-cohesion of the pictorial layer. Considering also that the pictorial layer can be heterogeneous at the μ-ATR scale, the resulting spectrum is liable to contain only the pigments’ absorptions (in pigment-binder systems). This is attributable to the formation of pigments aggregates, poor in binder, and hard enough to contrast the crystal pressure. More elastic binders such as EY, on the other hand, create a flexible film, which bends under the crystal’s pressure, without fracturing, so that the resulting spectrum is representative of both binder and pigment. In most cases, this problem is overcome by ER-FTIR, which requires no contact with the sample, so that the spectra collected are fully representative of the entire pictorial layer.
The study of slightly more complex systems, made up of individual pigments or binary mixtures bound in one of the four binders and then painted on parchment, was mainly aimed at establishing the possible effects of each pigment on the position and/or the type of distortion of the marker bands identified for each binding medium. Blue, white, green, yellow and red mineral pigments containing carbonates, sulphates, silicates and oxides, were thoroughly characterized; bands assignments based on literature data [2, 13,14,15] are reported in Table 1.
As discussed, the region between 1900 and 1500 cm−1 is the main region of interest for the GA, EY, EW and WE marker bands. The binder’s identification is quite straightforward when the system contains pigments such as oxides (minium, lead–tin yellow), silicates (earths, smalt, natural and French ultramarine) or sulphides (vermillion). These compounds only show absorptions below about 1000 cm−1, and the spectra collected on the paintouts are quite similar to those of the pure binders (e.g. Fig. 3a–c). However, when the paint layer contains carbonate-based pigments, the spectral region between 1900 and 1500 cm−1 appears drastically affected by the pigment’s main absorption. In fact, as results of the strong absorption coefficient of the ν3(CO 3 = ), carbonate-containing paintouts usually show spectra dominated by an intense and broad inverted band in the 1500–1400 cm−1 region. Moreover, if the surface is sufficiently rough, the volume reflection, RV, increases the intensity of the ν1 + ν4 combination band, whose position can interfere with the C=O asymmetric stretching of lipids. As illustrated in Fig. 3d in the case of chalk, the spectrum is dominated by the pigment’s characteristic absorption and the discrimination between GA and egg-based binders is rather difficult. Only the lipid fraction is detectable by the C=O stretching. In that series of paintouts, the presence of a proteinaceous binder can only be inferred by the presence of N–H stretching (Fig. 2b). In the lead white paintouts (Fig. 3e), EW and WE show really close spectral features because of the presence of the pigment’s ν1 + ν4(CO 3 = ) combination band at 1740 cm−1. The ν(C=O) contribution is hidden and the ν(N–H) one is similar in both cases, making the discrimination between the two binders virtually impossible. Differently from the chalk-containing paintouts, in the lead white system the presence of GA can be hypothesized by the presence of a broad δ(OH) feature.
The region of combination and overtone bands, lying between 6500 and 3500 cm−1, cannot be considered diagnostic for binders in most of the cases studied here. Only pure EY can be identify by ν + δ(CH) combination bands. In general, due to the complexity of the investigated systems, that region often contains signals generated by the superposition of combination/overtone bands due to the various components of the pictorial layer. This is particularly true when paintouts contain azurite, and in some cases malachite, mixed with EY or WE. The 3ν3(CO 3 = ) and ν + δ(OH) absorptions of both copper carbonates are very close to the ν + δ(CH) combination bands of the lipid fraction, and the resulting overlap makes the binder’s bands barely distinguishable (Fig. 3f). Interestingly, however, this same spectral region can be used to identify lipid-containing binders, even in the presence of copper carbonates, using fiber optic reflectance spectroscopy (FORS) systems operating in the visible and near-infrared range (up to 2500 nm, corresponding to 4000 cm−1) .
Considering the evidence provided by these results, the best chances for a clear identification of the paint binder used in real manuscript illuminations are tied to the possibility of collecting spectra in areas painted with simple oxide and sulphide-based pigments such as minium, orpiment and vermillion, all three of which were used extensively by medieval and Renaissance illuminators. This is particularly true when the pictorial layer is thick enough to (at least partially) hide the parchment’s spectral contribution and/or when the paint layer has not been modelled with white carbonates.
Results and discussion: case studies
The practical benefits of using ER-FTIR to study illuminated manuscripts can be best illustrated by a few case studies, all relative to objects in the collection of the Fitzwilliam Museum in Cambridge, UK. The main goal of the analysis was the identification of the binder(s) used to paint each illumination. In some cases, we were also hoping to obtain results that would support the identification of pigments, based on previous analyses by means of other non-invasive methods such as X-ray fluorescence (XRF) and fibre-optics reflectance spectroscopy (FORS) . The three case studies discussed here show how ER-FTIR can often, although not always, be used to answer this type of research questions.
A fifteenth-century leaf by Jean Bourdichon
A late fifteenth-century leaf from a Book of Hours, painted by the workshop of renowned French artist Jean Bourdichon (Cambridge, Fitzwilliam Museum, Marlay Cutting Fr. 5, Fig. 4a), was analysed with the aim of identifying the paint binder used and to confirm the nature of the blue and green pigments.
ER-FTIR analysis provided a good spectral match between the spectra collected on several areas of the fragment and the pure GA reference and/or the paintouts with pigments bound in GA (e.g. see Fig. 4c). The presence of gum Arabic in an illuminated fragment of this period and origin is expected.
The IR spectrum collected on the green garment (Fig. 4b) shows the typical shape of an absorption spectrum, without significant distortions except for some reststrahlen bands at low wavenumbers. The presence of natural ultramarine is clearly recognizable from the sharp signal at 2343 cm−1, together with an inverted band at 1021 cm−1. The presence of the sharp absorption at 2342 cm−1, due to the CO2 entrapped in the sodalite cage , is typical of the natural pigment. On the contrary, the synthetic one, the so called French ultramarine, does not show this absorption. The analysis of the higher wavenumbers spectral region (above 4000 cm−1) reveals the presence of two sharp absorptions, centred at 4380 and 4242 cm−1 respectively, which are definitive indicators of the presence of azurite. These signals are due both to an overtone (3ν3 CO 3 = ) and to the combination of the OH− stretching and bending. Interestingly, analysing the region of interest between 2600 and 2500 cm−1, we detected no signals that could clearly be assigned to the typical ν(CO3) combination bands of azurite. The green colour appears therefore to be a complex mixture of blue and yellow pigments, i.e. azurite, ultramarine and possibly lead–tin yellow. The presence of four inverted absorption bands at 562, 504, 459 and 427 cm−1 could suggest the use of lead–tin yellow type I. The position of these bands is slightly shifted compared to literature data  but XRF mapping carried out on this same manuscript fragments identified the presence of both tin and lead in green areas (P. Ricciardi, unpublished technical report), confirming the use of this pigment. Further analysis of the spectrum shows the presence of additional components in this complex mixture, in the form of two white pigments/extenders. The broad absorption at 2516 cm−1, showing a shoulder at 2594 cm−1, together with the well-defined shoulder at 1795 cm−1, can be attributed to the ν(CO3) combination bands in CaCO3. The presence of calcium carbonate is also supported also by the weak inverted signal at ≈ 1414 cm−1, due to the ν3 asymmetric stretching. The absorption bands which can be observed in the 2300–2000 cm−1 range can be ascribed to the combination and overtones band of SO 4 = in calcium sulphate. Unfortunately, due to the complexity of the spectrum, an unambiguous attribution to a precise calcium sulphate, i.e. gypsum, anhydrite or bassanite, is not possible. The presence of weak but sharp absorptions in the OH stretching region might suggest gypsum, CaSO4·2H2O, as the most likely candidate.
The spectrum collected on the blue robe (Fig. 4c) shows the presence of natural ultramarine as the blue pigment. The spectral bands of gypsum and calcite can also be easily recognized, in the region of interest from 2600 to 2000 cm−1. Gypsum is also present in the pink robe (Fig. 4d), as both its overtones and the main vibrational mode are easily detectable. In the region of interest between 2400 and 2000 cm−1 all the combination and overtone bands were identified together with the inverted ν3(1149 cm−1) and ν3(671 and 597 cm−1) bands. Moreover the O–H stretching shows a derivative-like band with an inflection point at 3410 cm−1. A weak signal due to CO 3 = group, probably CaCO3, was identified at 2517 cm−1. The Virgin’s veil (Fig. 4e) contains lead white. Overtone and combination bands due to carbonate group In hydrocerussite were easily detected at 1738 cm−1 (ν1 + ν4) and at 2421 cm−1 (2ν2 + ν4) together with ν3, affected by reststrahlen effect) and ν4, which shows a derivative like feature. Weak signals due to the SO 4 = overtones in gypsum and CO 3 = in calcium carbonate were also identified. Lead white also appears to be one of the constituents of the dark background (T5).
An eleventh-century Gospel Book
A page from an eleventh-century Gospel Book made in Bavaria (Cambridge, Fitzwilliam Museum, MS McClean 20, fol. 20v, Fig. 5a) was analysed with the main goal to determine the paint binder used by the artist. All the spectra collected on the page are characterised by similar absorptions in the 1800–1500 cm−1 region. Among these, the ones centred at 1678 and 1556 cm−1 can be ascribed to the A I and A II bands in proteinaceous binders, such as EW or WE. The use of a pure proteinaceous binder in the majority of the illumination, can be assumed by the absence of methylene ν + δ combination bands. Only in the pink robe (T1) and in the floral border decoration (T5) the spectral analysis reveals the use of a lipidic binder in combination with a proteinaceous one (Fig. 5b). Both spectra show, in addition to the typical amide bands, also two weak absorptions at ≈ 4334 and ≈ 4256 cm−1, ascribable to the above mentioned combination bands. Concerning the inorganic components of the pictorial layer, absorptions due to CO 3 = group were detected in all examined areas. In particular T1, T2, T3 and T5 shows the typical absorption of hydrocerussite, with the main vibration bands ν3, ν4 and νOH of Pb3(CO3)3(OH)2 clearly detectable at ≈ 1415, 690 and 3566 cm−1 (Fig. 5b). Tn T2 and T3, lead white is presence in association with natural ultramarine, clearly identifiable by its distinctive ν(CO2) absorption (Fig. 5b). In green areas (T5–7), although XRF shows the presence of Cu as the main chromophore, no signals ascribable to malachite are detected. These spectra instead show several distinctive absorptions, at 4074, 3452, 3388 and 1982 cm−1, together with three distinct inverted bands, at 584, 508 and 439 cm−1 (Fig. 5c). These bands can be associated with atacamite, Cu2Cl(OH)3 . In particular, the lower wavenumber bands are ascribable to the Cu–O stretching mode, while the ones at 3452 and 3388 cm−1 correspond to the OH stretching modes. The two bands at 4074 and 1982 cm−1 could be assigned to overtone and/or combination bands of the Cu–Cl and Cu–OH normal modes.
A Flemish Book of Hours
The analysis of two images on an early sixteenth century Flemish Book of Hours (Cambridge, Fitzwilliam Museum, MS 1058–1975, fols. 13v-14r) revealed an interesting difference in the pigments used on the two pages, despite the fact that they face each other in the manuscripts and have long been attributed to the same artist. The measurements performed on fol 13v (Fig. 6a) are dominated by the absorptions of carbonate groups. With the exclusion of the spectrum collected on the blue background (T2), all the spectra show a complex superimposition of distorted bands in the 1800–1300 cm−1 region. The complexity of that region arises from the partial overlap between the (ν1 + ν4) CO 3 = overtone, enhanced by the RV, and an absorption at ≈ 1684 cm−1. The latter, affected by a derivative-like distortion, can be attributed to the A I stretching of a proteinaceous binder. In almost all the spectra, A II (at ≈ 1582 cm−1), is partially hidden by the intense and broad inverted band due to the ν3 of CO 3 = group. The absence of methylene ν + δ combination bands suggests the use of a purely proteinaceous medium such as EW. Concerning the carbonate-containing pigments, chalk predominates in grey areas (T1) whereas azurite is present in blue ones (T2). The T1 spectrum is dominated by the intense ν3(1411 cm−1) together with ν1 + ν4(1796 cm−1) and ν1 + ν3 and/or 2ν2 + ν4(2514 cm−1) absorptions of calcium carbonate. Intense bands of azurite are well detectable in the spectrum T2 (Fig. 6c). The ν(OH) with inflection point at 4442 cm−1, with its typical derivative-like feature, is attributable to the hydroxyl groups in Cu3(CO3)2(OH)2. A reststrahlen band related to ν3 in carbonate group is clearly identifiable also in the green jewel (T3, Fig. 6d). Unexpectedly, however, it is not associated to malachite or azurite but, once again, to calcite, with overtones and combination bands of CaCO3 detectable at 1795 (ν1 + ν4) and 2514 (ν1 + ν3 and/or 2ν2 + ν4) cm−1 respectively. Excluding the presence of copper carbonates, the nature of the green colour has therefore still to be clarified. Considering the region of interest towards the near infrared, a peculiar broad absorption peak is detectable at 4276 cm−1, exhibiting a shoulder at 4423 cm−1. According to literature data , the presence of these two signals, together with a weak absorption at 3533 cm−1 and with an inverted band at 1081 cm−1, can be assigned to brochantite, a green copper sulphate (CuSO4∙3Cu(OH)2). Calcium carbonate is the predominant signal in the flesh tone area (T4), and it coexists with gypsum in the pink border decoration (T6).
On fol. 14v (Fig. 6b), the binder also seems to be a proteinaceous one, likely the same one used on the previous page, as suggested by the presence of two intense bands, attributable to amide I and amide II (Fig. 6e), in spectra T’1 to T’5. A difference can however be found in the blue and green pigments used. Analysis of the peacock features reveals the presence of smalt and malachite, respectively, rather than the azurite and brochantite identified on fol. 13v. Malachite can be identified on the basis of the evident absorption at 4158 cm−1, due to the combination of the stretching and bending mode of the OH group, together with the CO 3 = combination bands ν1 + ν3 and/or 2ν2 + ν4, at 2536 and 2428 cm−1 and ν1 + ν4 at 1802 cm−1. Smalt is clearly present in the blue centre of the feather (T’2 and T’4, Fig. 6e) and identifiably by not only a broad inverted νSiO absorption at 1072 cm−1, but also an inverted one at 443 cm−1 attributable to metal-O bonds in the glassy matrix of this pigment. All of these spectra actually show evidence for the presence of both pigments, albeit in small quantities (e.g. traces of malachite in T’2, traces of smalt in T’1), due to the relatively large size of the areas analysed using the present set-up.
This paper confirms ER-FTIR as a powerful tool to study both paint binders and pigments in manuscript illuminations in a completely non-invasive way. The results obtained on the pure binders paintouts show that the discrimination between gum Arabic and egg-based binders is possible and easily achievable. Additionally, due to its lipidic content, egg yolk is distinguishable from egg white. Whole egg, however, can easily be confused with both EY and EW, depending on the amount of lipidic fraction actually present in the specific objects. The identification of inorganic pigments, mixed with different binders, is quite straightforward, thanks to the enhancement of overtones and combination bands by the RV. In the same paintouts, the distinction among different binders is strongly connected with the pigment typology and with the optical properties of the pictorial layer. We observe that oxides, silicates and sulphides do not strongly affect the binders’ spectral features. On the contrary, carbonate-containing pigments can seriously interfere with the discrimination of the paint medium. Generally speaking, however, carbonate pigments bound in GA can be discriminated from the same ones mixed with egg-based binders. Still, the ν + δ overtone in lipid can be useful to discriminate EY/WE from EW, although the distinction is rather difficult when malachite or azurite are mixed with EW because their combination bands can overlap the above-mentioned lipid marker. Investigations performed on illuminated manuscript fragments and bound volumes allowed the identification of both binders and pigments. Accurate spectral interpretation allowed the identification of different binders in different parts of the same illumination. Moreover the presence of relatively unusual Cu-based pigments such as atacamite and brochantite was revealed.
attenuated total reflectance
external-reflectance Fourier-transform infrared spectroscopy
fibre-optics reflectance spectroscopy
Fourier-transform infrared spectroscopy
X-ray fluorescence spectroscopy
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LN collected, elaborated and interpreted the infrared spectra with assistance from PR. LN and PR wrote the present manuscript. Both authors read and approved the final manuscript.
The authors wish to thank Dr. Spike Bucklow for preparing the paintouts. Dr. Stella Panayotova is gratefully acknowledged for allowing access to the illuminated manuscripts and providing art-historical background.
The authors declare that they have no competing interests.
Availability of data and materials
The datasets analysed during the current study are available from the corresponding author on reasonable request.
Partial funding for this research was provided by the University of Cambridge’s Returning Carers Scheme.
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